'Zwicky's Nonet': a compact merging ensemble of nine galaxies and 4C 35.06, a peculiar radio galaxy with dancing radio jets

作者：Biju K G^*; Bagchi Joydeep^*; Ishwara Chandra C H; Pandey Pommier M; Jacob Joe; Patil M K; Kumar P Sunil; Pandge Mahadev; Dabhade Pratik; Gaikwad Madhuri; Dhurde Samir; Abraham Sheelu; Vivek M; Mahabal Ashish A; Djorgovski S G

来源：Monthly Notices of the Royal Astronomical Society, 2017, 471(1): 617-628.

DOI：10.1093/mnras/stx1476

• galaxies: clusters: individual: Abell 407
• galaxies: elliptical and lenticular, cD
• galaxies: jets
• quasars: supermassive black holes
• radio continuum: galaxies

We report the results of our radio, optical and infrared studies of a peculiar radio source 4C 35.06, an extended radio-loud active galactic nucleus (AGN) at the centre of galaxy cluster Abell 407 (z = 0.047). The central region of this cluster hosts a remarkably tight ensemble of nine galaxies, the spectra of which resemble those of passive red ellipticals, embedded within a diffuse stellar halo of similar to 1 arcmin size. This system (named 'Zwicky's Nonet') provides unique and compelling evidence for a multiple-nucleus cD galaxy precursor. Multifrequency radio observations of 4C 35.06 with the Giant Meterwave Radio Telescope (GMRT) at 610, 235 and 150 MHz reveal a system of 400-kpc scale helically twisted and kinked radio jets and outer diffuse lobes. The outer extremities of jets contain extremely steep-spectrum (spectral index -1.7 to -2.5) relic/fossil radio plasma with a spectral age of a few x (10(7)-10(8)) yr. Such ultra-steep spectrum relic radio lobes without definitive hotspots are rare and they provide an opportunity to understand the life cycle of relativistic jets and physics of black hole mergers in dense environments. We interpret our observations of this radio source in the context of growth of its central black hole, triggering of its AGN activity and jet precession, all possibly caused by galaxy mergers in this dense galactic system. A slow conical precession of the jet axis due to gravitational perturbation between interacting black holes is invoked to explain the unusual jet morphology.

• 出版日期2017-10